Cuby, Jean-GabrielJean-GabrielCubyOesch, PascalPascalOeschCooray, AsanthaAsanthaCoorayRhodes, JasonJasonRhodesBremer, MalcomMalcomBremerBowler, RebeccaRebeccaBowlerCapak, P.P.CapakCaputi, KarinaKarinaCaputiCASTELLANO, MARCOMARCOCASTELLANOConselice, ChristopherChristopherConseliceCuillandre, Jean-CharlesJean-CharlesCuillandreDayal, PratikaPratikaDayalDavidzon, IaryIaryDavidzonDunlop, JamesJamesDunlopFinkelstein, StevenStevenFinkelsteinFONTANA, AdrianoAdrianoFONTANAKashlinsky, AlexanderAlexanderKashlinskyKoopmans, LeonLeonKoopmansKuijken, KonradKonradKuijkenLe Brun, VincentVincentLe BrunLe Fèvre, OlivierOlivierLe FèvreMortlock, DanielDanielMortlockPello, RoserRoserPelloPENTERICCI, LauraLauraPENTERICCISahlén, MartinMartinSahlénSCHNEIDER, RAFFAELLARAFFAELLASCHNEIDERSerjeant, StephenStephenSerjeantWarren, StephenStephenWarren2021-02-082021-02-0820192330-9458http://hdl.handle.net/20.500.12386/30237Euclid and WFIRST will find thousands of galaxies and quasars above redshift 7 during the epoch of reionization. Massive spectroscopic follow-up campaigns with existing and planned near-infrared and mm facilities will be required for confirmation and physical characterization. A properly coordinated large follow-up campaign is recommended.ELETTRONICOenArticlehttps://baas.aas.org/pub/2020n3i360/release/12019BAAS...51c.360CFIS/05 - ASTRONOMIA E ASTROFISICA